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• W1971167288 abstract "We present high angular resolution (1″.2), narrow-band (Δλ/λ=0.1) images of the nucleus of NGC 253 at three wavelengths in the mid-infrared (8.5, 10.0, and 12.5 μm). We find that most of the mid-IR flux in the nucleus of NGC 253 derives from a very small region ≤120 pc in diameter. Within this small region there are three spatially and spectrally distinct IR components: two bright compact sources, and a surrounding envelope of low-level, diffuse emission. The mid-IR and 6 cm radio are loosely correlated in position but not in brightness. The implication is that the mid-IR-radio correlation may begin to break down on small spatial scales relevant to individual star-forming regions and large individual sources" @default.
• W1971167288 created "2016-06-24" @default.
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• W1971167288 date "1993-08-01" @default.
• W1971167288 modified "2023-09-25" @default.
• W1971167288 title "The mid-infrared radio correlation at high angular resolution - NGC 253" @default.
• W1971167288 doi "https://doi.org/10.1086/186950" @default.
• W1971167288 hasPublicationYear "1993" @default.
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